Chelen Johnson
Hertzsprung-Russel diagram for Active Galactic Nuclei (HR4AGN): Using space and ground based ultraviolet, optical, and infrared images to find a correlation between the color and luminosity of gas emission and dust emission around supermassive black holes at the centers of galaxies.
Every time we meet or talk or work on the project I feel just a little bit more knowledgeable, skilled and, perhaps most importantly, confident in what I know and can do...
I’ve already made big changes to my curriculum because of this program, and will continue to do so in future years.
One of the most interesting things I learned while working with my team was how unique and surprising each star can be.
